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- W1749192723 abstract "We outline the phenomenon of deep crustal heating in transiently accreting neutron stars. It is produced by nuclear transformations (mostly, by pycnonuclear reactions) in accreted matter while this matter sinks to densities rho > 10^{10} g/cc under the weight of freshly accreted material. We consider then thermal states of transiently accreting neutron stars (with mean mass accretion rates dot{M}=(10^{-14}-10^{-9}) M_odot/yr) determined by deep crustal heating. In a simplified fashion we study how the thermal flux emergent from such stars depends on the properties of superdense matter in stellar interiors. We analyze the most important regulators of the thermal flux: strong superfluidity in the cores of low-mass stars and fast neutrino emission (in nucleon, pion-condensed, kaon-condensed, or quark phases of dense matter) in the cores of high-mass stars. We compare the results with observations of soft X-ray transients in quiescent states." @default.
- W1749192723 created "2016-06-24" @default.
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- W1749192723 date "2002-11-05" @default.
- W1749192723 modified "2023-09-27" @default.
- W1749192723 title "Pycnonuclear burning and accreting neutron stars" @default.
- W1749192723 hasPublicationYear "2002" @default.
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